The production of light nuclei has attracted attention already at
lower incident energies in heavy-ion collisions at the AGS, SPS,
and RHIC [1]}, [2]}, [3]}.
A study of the dependence on \(\sqrt{s_{\mathrm {NN}}}\)  is of particular interest, because
different production mechanisms might dominate at various energies,
e.g. a formation via spectator fragmentation at lower energies or
via coalescence/thermal mechanisms at higher ones.
In all cases, an exponential drop in the yield was found with
increasing mass of the
nuclei [4]}, [5]}.
At RHIC and now at the LHC,
matter with a high content
of strange and of anti-quarks is created in heavy-ion
collisions. This has led to the first observation of
anti-alphas [6]}
and of anti-hypertritons [7]}. Their yields at LHC
energies were predicted based on thermal model estimates
in [8]}, [9]}.
